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Supernova Cooling in a Dark Matter Smog

Zhang, Yue (2014) Supernova Cooling in a Dark Matter Smog. Journal of Cosmology and Astroparticle Physics, 2014 (11). Art. No. 042. ISSN 1475-7516. http://resolver.caltech.edu/CaltechAUTHORS:20140512-094346126

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Abstract

A light hidden gauge boson with kinetic mixing with the usual photon is a popular setup in theories of dark matter. The supernova cooling via radiating the hidden boson is known to put an important constraint on the mixing. I consider the possible role dark matter, which under reasonable assumptions naturally exists inside supernova, can play in the cooling picture. Because the interaction between the hidden gauge boson and DM is likely unsuppressed, even a small number of dark matter compared to protons inside the supernova could dramatically shorten the free streaming length of the hidden boson. A picture of a dark matter "smog" inside the supernova, which substantially relaxes the cooling constraint, is discussed in detail.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1404.7172arXivDiscussion Paper
http://dx.doi.org/10.1088/1475-7516/2014/11/042 DOIArticle
http://iopscience.iop.org/1475-7516/2014/11/042/PublisherArticle
Additional Information:© 2014 IOP Publishing. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Article funded by SCOAP3. Received November 4, 2014; Accepted November 15, 2014; Published November 27, 2014. I would like to thank Haipeng An, Clifford Cheung, Rabi Mohapatra, Goran Senjanović, Mark Wise and Haibo Yu for useful discussions, and especially Shmuel Nussinov on illuminating conversation on the back reaction on dark matter in the supernova. This work is supported by the Gordon and Betty Moore Foundation through Grant No. 776 to the Caltech Moore Center for Theoretical Cosmology and Physics, and by the DOE Grant DE-FG02-92ER40701.
Group:Caltech Theory, Moore Center for Theoretical Cosmology and Physics
Funders:
Funding AgencyGrant Number
Gordon and Betty Moore Foundation776
Department of Energy (DOE)DE-FG02-92ER40701
SCOAP3UNSPECIFIED
Subject Keywords:dark matter theory; core-collapse supernovas
Classification Code:PACS: 95.35.+d; 97.60.Bw; 14.70.Pw; 95.30.Cq
Record Number:CaltechAUTHORS:20140512-094346126
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140512-094346126
Official Citation:Supernova cooling in a dark matter smog Yue Zhang JCAP11(2014)042
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45670
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:12 May 2014 16:52
Last Modified:14 Jun 2018 22:55

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